Parent article: NIRSpec Instrumentation
NIRSpec is sensitive to nearly a full decade in wavelength: 0.6–5.3 µm. The NIRSpec optical path contains two wheel mechanisms, the filter wheel assembly (FWA) and the grating wheel assembly (GWA), which provide disperser-filter combinations to cover the NIRSpec wavelength range. The NIRSpec filters and dispersers form matched sets to cover the wavelength ranges shown in Figure 1, with one configuration in low spectral resolution mode (R ~ 30 - 300), and four configurations in medium (R ~ 1000) and high (R ~ 2700) spectral resolution mode.
The FWA contains seven transmission filters, plus an OPAQUE position. The GWA contains six diffraction gratings, a double-pass prism, and a flat mirror.
Figure 1. NIRSpec wavelength coverage
A pictorial representation of the NIRSpec wavelength coverage and the number of configurations necessary to cover the full ~0.6–5.3 µm spectral range in the low, medium and high spectral resolution settings.
NIRSpec's seven transmission filters are: F140X, F110W, F070LP, F100LP, F170LP, F290LP, and CLEAR. Four of the filters are long-pass filters, i.e., they have a well defined cut-on wavelength and transmit all longer wavelengths. The other three filters are bandpass filters, with both a cut-on and cut-off wavelength, and are mainly used for target acquisition, or with the prism. Table 1 summarizes the properties of the transmission filters, and Figure 2 shows their optical throughput. The LP and CLEAR filters are matched with gratings to define the wavelength regions used for NIRSpec science.
There is also an eighth NIRSpec FWA position, OPAQUE, that is used as an instrument shutter. It blocks light from entering NIRSpec during calibration exposures and whenever NIRSpec is not being used.
Table 1. Transmission filters
|F140X1||0.8 to 2.0||target acquisition|
|F110W||1.0 to 1.3||narrowband acquisition for brighter targets|
|F070LP||>0.7||0.7 to 1.3 µm spectra|
|F100LP||>1.0||1.0 to 1.9 µm spectra|
|F170LP||>1.7||1.7 to 3.2 µm spectra|
|F290LP||>2.9||2.9 to 5.3 µm spectra |
|CLEAR||0.6 to 5.3||target acquisition or for use with PRISM|
|PageWithExcerpt||MR:APT GUI footnote|
Figure 2. Transmission filter throughput
The optical throughput of each of the NIRSpec transmission filters. The top plot shows the filters used for science spectral configurations. The bottom plot shows F110W and F140X, which are the filters for NIRSpec target acquisition. Users are strongly encouraged to use the ETC to make and compare source S/N estimates rather than attempt to model these independently. However, the system throughput curves (a component of which is the filter transmission) are available for download from the JWST ETC.
NIRSpec has seven dispersers in the GWA:
- three high resolution, R ~ 2,700, gratings (G140H, G235H, and G395H)
- three medium resolution, R ~ 1,000, gratings (G140M, G235M, and G395M)
- a low resolution, R ~ 100, double-pass prism (PRISM)
The full wavelength range of NIRSpec can be sampled in one exposure using the prism. However, each diffraction grating can only provide clean spectra over a factor of two in wavelength due to order contamination. The second order λ/2 spectra end up on exactly the same detector pixels as photons with wavelength λ (albeit with reduced efficiency). As a result, when using the diffraction gratings the wavelength limit on the short side (blueward) is defined by the throughput of the long pass filters, and the limit on the long side (redward) is defined by the wavelength where second-order light contaminates the spectrum. To obtain data over the entire 0.6–5.3 µm wavelength range using the gratings, spectra over smaller wavelength ranges are obtained using matched dispersers and filters, and then combined.
To avoid order contamination, each disperser is only used with its paired transmission filter(s), as shown in Table 2. Also shown are each combined grating-filter wavelength range and the nominal resolving power, which is defined as the resolving power at the center of the nominal wavelength range. Grating transmissions for the NIRSpec medium and high resolution dispersers are presented in Figure 3, and the wavelength dependence of the resolving powers is shown in Figure 4.
The last position in the GWA is a plane mirror, which provides undispersed imaging of the sky and is only used for target acquisition or field position verification during science operations.
Table 2. Available disperser-filter combinations
|Disperser-filter combination||Nominal resolving power||Wavelength range † |
|margin||15px 0 10px 0|
† Wavelength range values presented here are approximate. Note that the nominal spectral ranges for medium and high-resolution dispersers may be shortened due to red-end detector cutoffs. The cutoff wavelengths depend on the target aperture location (slit or shutter). Detailed limits are found on the wavelength ranges and gaps pages for the IFU, FS, and BOTS, and in the ETC. Information on wavelength ranges for MOS, which depend on the position of the shutter in the MSA, can be determined using the MSAViz Tool.
Figure 3. Transmission curves of the NIRSpec dispersers
The transmission curves of the NIRSpec dispersers as a function of wavelength. The top plot shows the transmission for the prism mode (R ~ 100), the middle plot shows the medium (R ~ 1,000) resolution dispersers and the bottom plot shows the transmission for the high (R ~ 2,700) resolution dispersers.
Figure 4. Resolving power of the NIRSpec dispersers
The resolving power of NIRSpec's gratings and prism as a function of wavelength. The resolving power is computed assuming a spectral resolution element size of 2.2 pixels (typically a fully illuminated aperture for the IFU, the MOS and the 200 mas slits). Note: The resolution for wider S1600A1 and S400A1 apertures may be degraded, especially for extended sources, but also for point sources at wavelengths long enough that the PSF width is > 2.2 pixels.
Dispersion curves for the NIRSpec dispersers
The dispersion and resolution curves as a function of wavelength for the different dispersers for the NIRSpec instrument are shown in Figures 5-11. Files containing the tabulated data used to produce these curves can be downloaded from the following links. These are binary fits tables that contain three columns: wavelength (micron), dispersion (microns/pixel) and resolution (λ⁄Δλ, unitless). These data are currently in use by the ETC (delivered June, 2016).
Figure 5. Dispersion and Resolution for the PRISM
Figure 6. Dispersion and Resolution for the G140M grating
Figure 7. Dispersion and Resolution for the G140H grating
Figure 8. Dispersion and Resolution for the G235M grating
Figure 9. Dispersion and Resolution for the G235H grating
Figure 10. Dispersion and Resolution for the G395M grating
Figure 11. Dispersion and Resolution for the G395H grating